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The general magnetic field of the sun, apparent variation of field-strength with level in the solar atmosphere

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1919 - 49 pagine

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Indice

Apparent Var1a
1
PAGE
34
The Orb1t of the Spectroscop1c B1nary Boss 46 Walter
51

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Parole e frasi comuni

2om exp absolute magnitude adopted apparent magnitude appear Astrophysical Journal average B-type B-type stars bipolar Boss brighter brightest calcium Cepheid variables Charlier cluster-type variables color color-curve color-index column of Table comparison stars components density derived determined diameter difference displacements distance equatorial segment faint fainter field-strength furnace galactic latitude galactic longitude galactic plane galactic system Galaxy giant stars given in Table globular clusters H fg Harvard indicated intensity km/sec light-curve lines of force luminosity luminosity-curve Maanen magnetic maximum measures median magnitude Messier 13 Milky Mount Wilson Mount Wilson Solar number of stars observed obtained open clusters parallaxes parsecs period photo-visual photographic magnitude polarity probable error proper motions radial velocities region relative Shapley spectra spectral types spectrum spots stellar sun-spot sun's systematic temperature tion variable stars variation vM fg vM g Wilson Contr Wilson Solar Observatory

Informazioni bibliografiche

QR code for The general magnetic field of the sun, apparent variation of field-strength with level in the solar atmosphere
TitoloThe general magnetic field of the sun, apparent variation of field-strength with level in the solar atmosphere
Edizione 148 di Contributions from the Mount Wilson Solar Observatory
AutoreGeorge Ellery Hale
pubblicato1919
Lunghezza49 pagine
  
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